The Standard Model Effective Field Theory (SMEFT) --- the EFT at the electroweak (EW) scale that realizes the EW symmetry linearly and obeys the gauge symmetry of the SM at higher energies without any new particles --- can be tested at low energies by identifying relations predicted by it among new physics Wilson Coefficients.
SMEFT predictions for semileptonic processes
Exploring observable effects of scalar operators beyond SMEFT ...
Identifying physics beyond SMEFT in the angular distribution of Lambdab decay ...
Coupling of ALPs with photons may lead to photons escaping optically opaque regions by oscillating into ALPs. This phenomenon may be viewed as the Light Shining through Wall (LSW) scenario in an astrophysical setting, and can be employed for appropriately chosen obscured magnetars.
Light Shining Through Wall Bounds on Axions From Obscured Magnetars
Ultralight scalar fields produced from their interactions with the intense EM fields near a compact star can have observable consequences such as change of photon dispersion relations and the spin-down rate of a binary system.
Constraining electromagnetic couplings of ultralight scalars from compact stars
Atmospheric neutrinos can act as a tool to probe the interior of Earth using weak interactions, and can provide information complementary to that obtained from gravitational and seismic measurements. While passing through Earth, multi-GeV neutrinos encounter Earth matter effects due to the coherent forward scattering with the ambient electrons, which alter the neutrino oscillation probabilities. These matter effects depend upon the density distribution of electrons inside Earth, and hence, can be used to determine the internal structure of Earth.
Constraining the core radius and density jumps inside Earth using atmospheric neutrino oscillations
Locating the core-mantle boundary using oscillations of atmospheric neutrinos
Probing dark matter inside Earth using atmospheric neutrino oscillations at INO-ICAL
Analytical expressions for the conversion probability of muon neutrino to electron neutrino were calculated in the presence of sterile neutrinos, with exact dependence on the sterile mass squared difference and matter effects. Experiments like DUNE have the ability to identify sterile mass ordering.
Sterile neutrinos: propagation in matter and sensitivity to sterile mass ordering
The effects of Lorentz violation and non-standard interactions of neutrinos can mimic each other in neutrino oscillations at long-baseline experiments. But observations of core-passing atmospheric neutrinos and antineutrinos can break this degeneracy.
A new perturbative technique was developed for analyzing physical situations where the effective Hamiltonian has non-commuting Hermitian and anti-Hermitian components, a situation that arises when neutrinos pass through matter.
Analytic treatment of 3-flavor neutrino oscillation and decay in matter
Neutrino Propagation When Mass Eigenstates and Decay Eigenstates Mismatch
The quantum nature of neutrino oscillations would be reflected in the mismatch between the neutrino survival probabilities with and without an intermediate observation. This ``quantum mismatch'' measure would complement the Leggett-Garg measure at long baseline experiments.
Quantum mismatch: A powerful measure of quantumness in neutrino oscillations